Abstract
In the previous section we have seen that, in the context of nV -fold, N = 2, d = 4 MESGT, the fundamental properties of 4-d extreme BHs may be described by the “BH effective potential” function V (z, z; p, q), and in particular by its critical points in the moduli space M z , z , which is endowed with a (regular) special Kähler geometry. New insights can be gained by considering the formalism of the geometric approach to the thermodynamical fluctuation theory. Once again, we will mainly follow Ferrara, Gibbons, and Kallosh [55] (for a complete review, see, e.g., [82]).
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 2006 Springer
About this chapter
Cite this chapter
Bellucci, S., Marrani, A., Ferrara, S. (2006). Black Hole Thermodynamics and Geometry. In: Supersymmetric Mechanics – Vol. 2. Lecture Notes in Physics, vol 701. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-34157-9_5
Download citation
DOI: https://doi.org/10.1007/3-540-34157-9_5
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-34156-7
Online ISBN: 978-3-540-34157-4
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)